VLBI for Gravity Probe B: The Guide Star IM Pegasi

We review the radio very long baseline interferometry (VLBI) observations of the guide star, IM Peg, and three compact extragalactic reference sources, 3C 454.3, B2250+194, and B2252+172, made in support of the NASA/Stanford gyroscope relativity mission, GP-B. The main goal of the observations was the determination of the proper motion of IM Peg relative to the distant universe. VLBI observations made between 1997 and 2005 yield a proper motion of IM Peg of -20.83 $\pm$ 0.09 mas yr$^{-1}$ in RA and -27.27 $\pm$ 0.09 mas yr$^{-1}$ in dec, in a celestial reference frame of extragalactic radio galaxies and quasars virtually identical to the International Celestial Reference Frame 2 (ICRF2). They also yield a parallax for IM Peg of 10.37 $\pm$ 0.07 mas, corresponding to a distance of 96.4 $\pm$ 0.7 pc. The uncertainties are standard errors with statistical and estimated systematic contributions added in quadrature. These results met the pre-launch requirements of the GP-B mission to not discernibly degrade the estimates of the geodetic and frame-dragging effects. The paper also reports on a 1$\sigma$ upper limit on the magnitude of the components of the proper motion of the 'core' of 3C 454.3 relative to the ICRF2 of 46 and 56 $\mu$as yr$^{-1}$ in RA and dec, respectively, and presents densely sampled ellipses of the parallax and the orbit of the giant of the binary system. It further gives a sequence of images of the flickering radio emission relative to the disk of the giant. For a 'movie of a star,' see http://www.yorku.ca/bartel/impeg.mpg .
Comment: Invited review accepted for publication in a Special Issue of Classical and Quantum Gravity, 27 pages, 9 figures, 3 tables